Abstract

Earth deformation at the diurnal tidal frequencies includes the resonant tidal-forcing response caused by the Free Core Nutation (FCN), a retrograde mode related to the slight misalignment of the rotation axes of the outer core and mantle. We analyse data from four underground high-sensitivity laser extensometers, whose signal-to-noise ratio in the diurnal tidal band is particularly high, and provide an alternative independent estimate of the FCN complex frequency with respect to more usual techniques (nutation and gravity). Firstly, we differentiate displacements due to diurnal solid tides to obtain extension along any azimuthal direction in terms of three complex parameters (A, S, C) which depend on latitude and frequency. Then, we demonstrate that we can invert the FCN complex frequency and the sensitivity of Im(A) and Re(S) to the resonance from our data. Lastly we obtain the probability distributions of those four parameters. Our results are in full agreement with those from nutation and gravity, as well as with reference IERS (International Earth Rotation and Reference Systems Service) values. Sensitivities of Im(A) and Re(S) to the resonance are estimated here for the first time and are in agreement with values computed using reference Love and Shida numbers from IERS.

Highlights

  • The Free Core Nutation (FCN) is a retrograde mode related to the slight misalignment of the rotation axes of the Earh’s fluid outer core and mantle, with a period TFCN ∼ 430 sidereal days in the celestial reference frame

  • Since fFCN falls inside the diurnal tidal band, the FCN causes a resonant response of some diurnal tides

  • Where σj are the resonance frequencies associated with the Chandler wobble (CW, j = 1), the FCN (j = 2), and the free inner core nutation (FICN, j = 3), σ and σj are expressed in cpsd, and all the parameters are complex

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Summary

Introduction

The Free Core Nutation (FCN) is a retrograde mode related to the slight misalignment of the rotation axes of the Earh’s fluid outer core and mantle, with a period TFCN ∼ 430 sidereal days in the celestial reference frame. Optimal model parameters are obtained through the comparison between the experimental data set and theoretical diurnal tides (Eqs. 3 and 4) corrected for ocean loading and siting effects (Eq 2).

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